GRB 220107A (red star) in the Amati (left) and Yonetoku (right) planes based on Konus-Wind data. The sample of Type I (short/hard; triangles) and Type II (long; circles) GRBs is taken from Tsvetkova et al. (2017, 2021), with points color-coded by redshift. The shaded regions denote the 1σ and 2σ scatter around the best-fit correlations. For GRB 220107A, we derive E_iso = (2.15 ± 0.08)×10⁵³ erg and (1 + z)E_p, i = (540 ± 34) keV from the time-integrated spectrum and L_iso = (7.86 ± 0.57)×10⁵² erg s⁻¹ with (1 + z)E_p, p = (425 ± 35) keV from the peak spectrum. Both measurements confirm that GRB 220107A lies in good agreement with the established Amati and Yonetoku relations.